CHESS – Constellation of CubeSats: Analyzing the drivers of the Earth’s exosphere with MS and GNSS

Chemical composition and density measurements of the upper atmosphere provide key insights into the origin and evolution of celestial objects. The density and the chemical composition of planet’s atmosphere may evolve from a hostile, dense primary atmosphere to a life‐harbouring tertiary atmosphere as present on Earth by losing atmospheric species to space upon formation of the object. The present-day atmospheric escape rates can be measured or inferred from exospheric temperatures and density profiles, for many species of the upper atmosphere. By modelling, these escape rates can be adapted to conditions in the past to study the evolution of the atmospheric composition.

The terrestrial exosphere and upper ionosphere are complex dynamic regions that adapt to several endogenous and exogenous drivers. The Sun as such a driver forces the upper atmosphere to respond to the solar UV/EUV flux and solar energetic particles. These external influences cause a variation of both the density, extent, and the chemical composition of the upper atmosphere on several time scales ranging from minutes to the age of the Solar System leading to various phenomena including atmospheric evolution and night-side transport of species. Although these interactions have been extensively studied over the past decades, the scientific community still lacks some basic measurements in the terrestrial upper atmosphere to derive the exospheric temperatures and its variation as a function of the corresponding drivers.

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